Results 21 to 30 of about 1,487,361 (366)

Three-dimensional interstellar dust reddening maps of the Galactic plane [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
We present new three-dimensional (3D) interstellar dust reddening maps of the Galactic plane in three colours, E(G-Ks), E(Bp-Rp) and E(H-Ks). The maps have a spatial angular resolution of 6 arcmin and covers over 7000 deg$^2$ of the Galactic plane for ...
B.-Q. Chen   +8 more
semanticscholar   +1 more source

The Canadian Galactic Plane Survey [PDF]

open access: yesThe Astronomical Journal, 2003
The Canadian Galactic Plane Survey (CGPS) is a project to combine radio, millimeter, and infrared surveys of the Galactic plane to provide arcminute-scale images of all major components of the interstellar medium over a large portion of the Galactic disk.
Steven J. Gibson   +19 more
openaire   +2 more sources

Prospects for detection of a galactic diffuse neutrino flux

open access: yesFrontiers in Astronomy and Space Sciences, 2022
A Galactic cosmic-ray transport model featuring non-homogeneous transport has been developed over the latest years. This setup is aimed at reproducing γ-ray observations in different regions of the Galaxy (with particular focus on the progressive ...
P. De La Torre Luque   +6 more
doaj   +1 more source

Position and Proper Motion of Sagittarius A* in the ICRF3 Frame from VLBI Absolute Astrometry

open access: yesThe Astronomical Journal, 2023
Sagittarius A* (Sgr A*) is a strong, compact radio source believed to be powered by a supermassive black hole at the galactic center. Extinction by dust and gas in the galactic plane prevents observing it optically, but its position and proper motion ...
David Gordon   +2 more
doaj   +1 more source

On a possible corrugation of the galactic plane [PDF]

open access: yesSymposium - International Astronomical Union, 1970
We have studied the rotation curve of the Galaxy at different heights below and above the equator. In the course of this work we noticed that the maximum brightness temperature of hydrogen oscillates around the galactic plane following a fairly sinusoidal pattern.
C. M. Varsavsky, R. J. Quiroga
openaire   +2 more sources

Decomposing the Origin of TeV–PeV Emission from the Galactic Plane: Implications of Multimessenger Observations

open access: yesThe Astrophysical Journal Letters, 2023
High-energy neutrino and γ -ray emission has been observed from the Galactic plane, which may come from individual sources and/or diffuse cosmic rays.
Ke Fang, Kohta Murase
doaj   +1 more source

GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey II: Galactic plane 345° < l < 67°, 180° < l < 240° [PDF]

open access: yesPublications Astronomical Society of Australia, 2019
This work makes available a further $2\,860~\text{deg}^2$ of the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey, covering half of the accessible galactic plane, across 20 frequency bands sampling 72–231 MHz, with resolution ...
N. Hurley-Walker   +18 more
semanticscholar   +1 more source

MeerGAL: the MeerKAT Galactic Plane Survey [PDF]

open access: yesProceedings of MeerKAT Science: On the Pathway to the SKA — PoS(MeerKAT2016), 2018
Radio surveys of the Milky Way galaxy have transformed our understanding of star formation\ud and stellar evolution. However, due to strong dependence of “survey cost” on frequency most\ud large area surveys have so far been carried out at low frequencies (? a few GHz).
Thompson, M. A.   +24 more
openaire   +5 more sources

On the galactocentric orbits of nearby stars [PDF]

open access: yesSerbian Astronomical Journal, 1999
Using the data from the Gliese-Jahreiss Catalogue and a particular form of the galactic potential the authors construct galactocentric orbits for nearby stars.
Ninković S., Popović N., Živkov V.
doaj   +1 more source

ARCADE 2 Observations of Galactic Radio Emission [PDF]

open access: yes, 2009
We use absolutely calibrated data from the ARCADE 2 flight in July 2006 to model Galactic emission at frequencies 3, 8, and 10 GHz. The spatial structure in the data is consistent with a superposition of free-free and synchrotron emission.
A. Kogut   +37 more
core   +3 more sources

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